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Indirect Solar Wind Measurements Using Archival Cometary Tail Observations. / Золотова, Надежда Валерьевна; Sizonenko, Yu.; Вохмянин, Михаил Владимирович; Veselovsky, I.

в: Solar Physics, Том 293, № 5, 85, 01.05.2018.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Золотова, НВ, Sizonenko, Y, Вохмянин, МВ & Veselovsky, I 2018, 'Indirect Solar Wind Measurements Using Archival Cometary Tail Observations', Solar Physics, Том. 293, № 5, 85. https://doi.org/10.1007/s11207-018-1307-4

APA

Золотова, Н. В., Sizonenko, Y., Вохмянин, М. В., & Veselovsky, I. (2018). Indirect Solar Wind Measurements Using Archival Cometary Tail Observations. Solar Physics, 293(5), [85]. https://doi.org/10.1007/s11207-018-1307-4

Vancouver

Золотова НВ, Sizonenko Y, Вохмянин МВ, Veselovsky I. Indirect Solar Wind Measurements Using Archival Cometary Tail Observations. Solar Physics. 2018 Май 1;293(5). 85. https://doi.org/10.1007/s11207-018-1307-4

Author

Золотова, Надежда Валерьевна ; Sizonenko, Yu. ; Вохмянин, Михаил Владимирович ; Veselovsky, I. / Indirect Solar Wind Measurements Using Archival Cometary Tail Observations. в: Solar Physics. 2018 ; Том 293, № 5.

BibTeX

@article{f6e6476bd298473399f0f651e6af7018,
title = "Indirect Solar Wind Measurements Using Archival Cometary Tail Observations",
abstract = "This paper addresses the problem of the solar wind behaviour during the Maunder minimum. Records on plasma tails of comets can shed light on the physical parameters of the solar wind in the past. We analyse descriptions and drawings of comets between the eleventh and eighteenth century. To distinguish between dust and plasma tails, we address their colour, shape, and orientation. Based on the calculations made by F.A. Bredikhin, we found that cometary tails deviate from the antisolar direction on average by more than 10∘10 degrees, which is typical for dust tails. We also examined the catalogues of Hevelius and Lubieniecki. The first indication of a plasma tail was revealed only for the great comet C/1769 P1.",
keywords = "солнечный ветер, кометы, Comets, Solar wind",
author = "Золотова, {Надежда Валерьевна} and Yu. Sizonenko and Вохмянин, {Михаил Владимирович} and I. Veselovsky",
note = "Funding Information: Acknowledgements The reported study was partially funded by RFBR according to the research project 16-02-00300-a. The work by I.S. Veselovsky in the Space Research Institute is supported by the grant RSCF 16-12-10062-a.",
year = "2018",
month = may,
day = "1",
doi = "10.1007/s11207-018-1307-4",
language = "English",
volume = "293",
journal = "Solar Physics",
issn = "0038-0938",
publisher = "Springer Nature",
number = "5",

}

RIS

TY - JOUR

T1 - Indirect Solar Wind Measurements Using Archival Cometary Tail Observations

AU - Золотова, Надежда Валерьевна

AU - Sizonenko, Yu.

AU - Вохмянин, Михаил Владимирович

AU - Veselovsky, I.

N1 - Funding Information: Acknowledgements The reported study was partially funded by RFBR according to the research project 16-02-00300-a. The work by I.S. Veselovsky in the Space Research Institute is supported by the grant RSCF 16-12-10062-a.

PY - 2018/5/1

Y1 - 2018/5/1

N2 - This paper addresses the problem of the solar wind behaviour during the Maunder minimum. Records on plasma tails of comets can shed light on the physical parameters of the solar wind in the past. We analyse descriptions and drawings of comets between the eleventh and eighteenth century. To distinguish between dust and plasma tails, we address their colour, shape, and orientation. Based on the calculations made by F.A. Bredikhin, we found that cometary tails deviate from the antisolar direction on average by more than 10∘10 degrees, which is typical for dust tails. We also examined the catalogues of Hevelius and Lubieniecki. The first indication of a plasma tail was revealed only for the great comet C/1769 P1.

AB - This paper addresses the problem of the solar wind behaviour during the Maunder minimum. Records on plasma tails of comets can shed light on the physical parameters of the solar wind in the past. We analyse descriptions and drawings of comets between the eleventh and eighteenth century. To distinguish between dust and plasma tails, we address their colour, shape, and orientation. Based on the calculations made by F.A. Bredikhin, we found that cometary tails deviate from the antisolar direction on average by more than 10∘10 degrees, which is typical for dust tails. We also examined the catalogues of Hevelius and Lubieniecki. The first indication of a plasma tail was revealed only for the great comet C/1769 P1.

KW - солнечный ветер

KW - кометы

KW - Comets

KW - Solar wind

UR - https://link.springer.com/article/10.1007%2Fs11207-018-1307-4

UR - http://www.scopus.com/inward/record.url?scp=85047477532&partnerID=8YFLogxK

U2 - 10.1007/s11207-018-1307-4

DO - 10.1007/s11207-018-1307-4

M3 - Article

VL - 293

JO - Solar Physics

JF - Solar Physics

SN - 0038-0938

IS - 5

M1 - 85

ER -

ID: 26941206